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UNIVERSITAT DE BARCELONA Departamen
- Page 5: Per a la meva neboda Blanca, que va
- Page 8 and 9: feina no presentada en aquesta tesi
- Page 10 and 11: desfogar-nos conjuntament, per la s
- Page 12 and 13: From the scientifical point of view
- Page 14 and 15: Gràcies a la meva germana Nàdia,
- Page 16 and 17: ii CONTENTS I Discovery and study o
- Page 18 and 19: iv CONTENTS II A search for new mic
- Page 20 and 21: vi CONTENTS
- Page 22 and 23: viii Resum de la tesi d’Eddington
- Page 24 and 25: x Resum de la tesi imprescindible p
- Page 26 and 27: xii Resum de la tesi dels sistemes
- Page 28 and 29: xiv Resum de la tesi un comportamen
- Page 30 and 31: xvi Resum de la tesi MilliARC SEC 4
- Page 32 and 33: xviii Resum de la tesi per poder de
- Page 34 and 35: xx Resum de la tesi valors força s
- Page 36 and 37: xxii Resum de la tesi 2. D’entre
- Page 38 and 39: xxiv Resum de la tesi pano Alemán
- Page 40 and 41: xxvi Resum de la tesi 3.3 Observaci
- Page 42 and 43: xxviii Resum de la tesi habitual en
- Page 44 and 45: xxx Resum de la tesi Per tant, si l
- Page 46 and 47: xxxii BIBLIOGRAFIA
- Page 48 and 49: 2 Chapter 1. Introduction and backg
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- Page 58 and 59: 12 Chapter 1. Introduction and back
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- Page 68 and 69: 22 Chapter 1. Introduction and back
- Page 70 and 71: 24 Chapter 1. Introduction and back
- Page 72 and 73: 26 Chapter 1. Introduction and back
- Page 74 and 75: 28 BIBLIOGRAPHY Lewin, W. H. G., va
- Page 76 and 77: 30 BIBLIOGRAPHY
- Page 79 and 80: Chapter 2 Multiwavelength approach
- Page 81 and 82: 2.3. An interesting target in the s
- Page 83 and 84: 2.4. The radio counterpart: NVSS J1
- Page 85 and 86: 2.4. The radio counterpart: NVSS J1
- Page 87 and 88: 2.4. The radio counterpart: NVSS J1
- Page 89 and 90: 2.4. The radio counterpart: NVSS J1
- Page 91 and 92: 2.4. The radio counterpart: NVSS J1
- Page 93 and 94: 2.4. The radio counterpart: NVSS J1
- Page 95 and 96: 2.4. The radio counterpart: NVSS J1
- Page 97 and 98: 2.4. The radio counterpart: NVSS J1
- Page 99 and 100: 2.4. The radio counterpart: NVSS J1
- Page 101 and 102: 2.5. The optical/IR star: LS 5039 5
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2.5. The optical/IR star: LS 5039 6
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2.5. The optical/IR star: LS 5039 6
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2.6. The X-ray counterpart: RX J182
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2.6. The X-ray counterpart: RX J182
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2.6. The X-ray counterpart: RX J182
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2.6. The X-ray counterpart: RX J182
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2.6. The X-ray counterpart: RX J182
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2.7. The γ-ray counterpart: 3EG J1
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2.7. The γ-ray counterpart: 3EG J1
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2.8. A proposed scenario to explain
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Figure 2.23: Scenario where the mul
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2.8. A proposed scenario to explain
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2.8. A proposed scenario to explain
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2.9. Conclusions 87 8. We have carr
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Bibliography Blandford, R. D., & K
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BIBLIOGRAPHY 91 Merck, M., Bertsch,
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Chapter 3 LS 5039 as a runaway micr
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3.1. Positions and proper motions 9
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3.1. Positions and proper motions 9
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3.3. The past trajectory of LS 5039
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3.4. SNR G016.8−01.1 101 DECLINAT
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3.4. SNR G016.8−01.1 103 Normaliz
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3.4. SNR G016.8−01.1 105 Galactic
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3.5. The H i surroundings of LS 503
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3.6. Discussion 109 experienced a h
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3.6. Discussion 111 At this point w
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3.7. Conclusions 113 6. Finally, th
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Bibliography Ankay, A., Kaper, L.,
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BIBLIOGRAPHY 117 Schaerer, D., de K
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Part II A search for new microquasa
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122 Chapter 4. The cross-identifica
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124 Chapter 4. The cross-identifica
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126 Chapter 4. The cross-identifica
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128 Chapter 4. The cross-identifica
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130 BIBLIOGRAPHY
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132 Chapter 5. Radio and optical ob
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DECLINATION (J2000) DECLINATION (J2
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136 Chapter 5. Radio and optical ob
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138 Chapter 5. Radio and optical ob
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140 Chapter 5. Radio and optical ob
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142 Chapter 5. Radio and optical ob
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144 Chapter 5. Radio and optical ob
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146 Chapter 5. Radio and optical ob
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148 BIBLIOGRAPHY
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150 Chapter 6. EVN and MERLIN obser
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152 Chapter 6. EVN and MERLIN obser
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154 Chapter 6. EVN and MERLIN obser
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156 Chapter 6. EVN and MERLIN obser
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158 Chapter 6. EVN and MERLIN obser
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160 Chapter 6. EVN and MERLIN obser
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162 Chapter 6. EVN and MERLIN obser
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164 Chapter 6. EVN and MERLIN obser
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166 BIBLIOGRAPHY
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General conclusions 171 Since each